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Dark Matter and Extragalactic Gas Clouds in the NGC 4532/DDO 137 SystemH I synthesis mapping of NGC 4532 and DDO 137, a pair of Sm galaxies on the edge of the Virgo cluster, is used to determine rotation curves for each of the galaxies and to resolve the structure and kinematics of three extragalactic H I clouds embedded in an extended envelope of diffuse HI discovered in earlier Arecibo studies of the system.
Document ID
20060041290
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hoffman, G. L.
Lu, N. Y.
Salpeter, E. E.
Connell, B. M.
Date Acquired
August 23, 2013
Publication Date
April 1, 1998
Publication Information
Publication: Astronomical Journal
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Other
Keywords
Dark Matter Extragalactic Gas Clouds mappinig

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